CMB Polarization with POLARBEAR
THE COSMIC MICROWAVE BACKGROUND AND COSMOLOGY
Over the last two decades, studies of the Cosmic Microwave Background (CMB) intensity anisotropies have provided precise measurements of the basic parameters that describe our universe.
Inflationary theories are currently the best framework we have to explain several aspects of the Universe today. They predict that the early Universe underwent a phase of exponential expansion during which a background of gravitational waves was produced. Those gravitational waves will then produce a primordial B-mode signal at the time of recombination. An inflationary phase would have occurred at such high energy density that there is no hope of studying the phenomena in any accelerator that could be built on earth. POLARBEAR, however, will be able to see the direct signature of Inflation through CMB polarization, and will potentially be able to investigate physics that occurs at energies where all the forces of nature are unified.
The evolution of the universe is based on the idea of gravitational instability, whereby initial tiny fluctuations in the density of the Universe grew under the influence of gravity to form the large-scale gravitational structures we see around us today. These structures bend the trajectories of CMB photons through gravitational lensing, distorting its primordial polarization and converting E-modes into B-modes. Imaging the lensing-generated B-modes, POLARBEAR will be able to shed light on all the components of the Universe influencing structure formation, such as neutrino mass and dark energy.